black-hole accretion

基本解釋

The single black hole-accretion disk precession model or disk-driven precession model is discussed carefully;
著重論述了單黑洞—吸積盤進動模型或盤致進動模型；
X-ray observations of iron in the accretion disks may actually be showing the effects of such a massive black hole as well.
同時，鐵的X射線對這種吸積現(xiàn)象的觀察資料實際上也可以反映這種巨大黑洞的影響。
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These two 'anti-quasars' provide special laboratories for us to study some of the dimmest type of accretion even seen onto a supermassive black hole.
李志遠說，“這兩個反類星體為我們提供了一個特殊的實驗室，去研究特大質(zhì)量黑洞的一些最模糊的一類增值?！?/li>

黑洞吸積
In this thesis I briefly introduce the definitions, classification, some observational characteristics of different black hole accretion models.
本文主要介紹了黑洞吸積的概念，分類以及對應(yīng)的光譜態(tài)特征，并對黑洞吸積各個模型，發(fā)展現(xiàn)狀等進行了綜述。